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DENSITY WAVES IN SATURN'S RINGS
Nov 10, 2004 - Researchers have used the Cassini spacecraft to make 
observations of Saturn's rings with tremendous clarity, resolving images down 
to the size of a football field. A team from the University of Colorado at 
Boulder have used a technique called "stellar occultation" to look through the 
rings at a distant star, and then watch how the ring particles obscure it. The 
ring material bunches up into denser areas, with gaps between them as small as 
50 metres (160 feet). This is unusual, because they should be spreading out in 
the vacuum of space - this means that small objects, like moons, are stirring 
up the material in the rings like ripples in a pond.

http://www.universetoday.com/am/publish/density_waves_saturn.html
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ICY OBJECTS COULD BE SMALLER THAN PREVIOUSLY THOUGHT
Nov 10, 2004 - Is Pluto a planet or just a really large Kuiper Belt Object 
(KBO)? Those arguing that it doesn't deserve planetary status will have to 
reconsider because of new research from the Spitzer Space Telescope. It was 
previously believed that KBOs were fairly dark, with a similar reflectivity to 
comets. From the reflectivity, astronomers guessed that KBOs are quite large, 
some getting as big as 700 km (434 miles) across. But new observations from 
Spitzer show that they're probably more reflective than previously thought, and 
therefore much smaller. This means that Pluto is probably still significantly 
larger than other objects in the Kuiper Belt.

http://www.universetoday.com/am/publish/icy_objects_smaller.html
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LAUNCH DATE SET FOR SOLAR SAIL
Nov 10, 2004 - The countdown has begun for the launch of the Planetary 
Society's Cosmos 1 spacecraft; the first ever to be powered by a solar sail. 
The privately built spacecraft will be lofted into orbit atop a Volna rocket on 
March 1, 2005. Once Cosmos 1 is in orbit, it will unfurl 8 triangular solar 
sails, and then use the sails to propel the spacecraft through the pressure of 
light from the Sun. Cosmos 1 wasn't designed for a long-term trip into space, 
so it's likely not to last too much longer than a few weeks, or months at the 
most, but it should serve as a working concept to help designers plan future 
spacecraft.

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X-RAY PORTRAIT OF PROXIMA CENTAURI
Nov 10, 2004 - NASA's Chandra X-Ray Observatory took this image of red dwarf 
star Proxima Centauri, our closest stellar neighbour (after the Sun, of 
course). The image shows that its surface is in a constant state of turmoil, 
with flares occurring almost continuously. Proxima Centauri has only 1/10th the 
mass of our own Sun, and the conversion of hydrogen to helium happens much more 
slowly. This creates turbulent, convective motion throughout its interior, 
which stores up magnetic energy - the energy is what creates all the flares.

http://www.universetoday.com/am/publish/xray_portrait_proxima.html
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A SOLAR SYSTEM'S ICY BUILDING BLOCKS
Nov 10, 2004 - New images released from the Spitzer space telescope are helping 
scientists understand how clouds of gas and dust come together to form new 
solar systems. One image shows a dim object at the heart of an icy cloud, which 
resembles our own early solar system. This object isn't a star... yet, but it 
could be a young failed star, a brown dwarf, a star which has yet to ignite, or 
something else entirely. In another image, Spitzer looked at the centre of a 
dusty disc around a young star and found icy building blocks that will 
eventually form into planets - similar to how our planets looked when they were 
only a few hundred thousand years old.

http://www.universetoday.com/am/publish/solar_systems_icy_building_blocks.html
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